Observation details report
Detailed source parameters (including errors) in a comma-separated values file
Click on source number for detailed analysis, including spectral fits if applicable
| data | idnum | idradec | telescope | instrument | x | y | cnts | cntserr | rate | rateerr | SNR | poisprob | sigmaj | sigmin | incang | offax | cnts_soft | cnts_hard | hr | hr_err | ext | var | N_H | flux | vign | flags | |
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| Report | 1 | X132607.28+074348.6 | chandra | ccd7 | 669.69 | 811.68 | 148.944 | 12.416 | 0.0298937 | 0.00249194 | 143.719 | 1 | 0.419195 | 0.349197 | 113.603 | 1.03338 | F | F | 1.85e+20 | 0 | 1 | ds | |||||
| Report | srcpi bgdpi arf | 4 | X132607.99+074022.8 | chandra | ccd7 | 648.252 | 393.452 | 78.3406 | 8.86885 | 0.0157233 | 0.00178001 | 75.5922 | 1 | 1.17749 | 0.543766 | 321.273 | 3.90786 | 47.8436 | 19.5699 | -0.419407 | 0.149703 | A | F | 1.86e+20 | 1.21546e-13 | 1 | dsx |
| Report | srcpi bgdpi arf | 2 | X132611.87+074358.6 | chandra | ccd7 | 531.186 | 831.941 | 48.2728 | 6.94786 | 0.00968855 | 0.00139446 | 46.5793 | 1 | 0.354776 | 0.354776 | 0 | 0.297217 | 33.9153 | 9.91533 | -0.547562 | 0.200501 | F | F | 1.85e+20 | 7.22705e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X132653.93+073930.3 | chandra | ccd3 | 617.087 | 412.055 | 32.9811 | 7.20991 | 0.00661944 | 0.00144706 | 10.6999 | 1 | 5.73867 | 1.86349 | 0.158017 | 11.6147 | 30.9827 | 1.21278 | -0.924661 | 0.296125 | F | F | 1.87e+20 | 9.71434e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 3 | X132601.79+074454.7 | chandra | ccd7 | 835.551 | 946.164 | 16.857 | 4.13996 | 0.00338326 | 0.000830906 | 16.2656 | 1 | 0.516836 | 0.516836 | 0 | 2.42 | 16.9152 | 0.830437 | -0.906407 | 0.407574 | F | F | 1.85e+20 | 2.64064e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 13 | X132624.62+073953.9 | chandra | ccd7 | 145.74 | 334.644 | 19.0583 | 4.36558 | 0.00382508 | 0.000876191 | 18.3897 | 1 | 1.94448 | 0.688883 | 335.554 | 5.45586 | 14.79 | 2.34005 | -0.72679 | 0.386732 | F | F | 1.86e+20 | 3.2146e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 10 | X132556.56+073744.5 | chandra | ccd7 | 993.375 | 71.25 | 9.58059 | 4.27872 | 0.00192285 | 0.00085875 | 14.7935 | 1 | 1.09253 | 0.492 | 163.059 | 7.40754 | 5.77123 | 1.92374 | -0.5 | 0.581176 | A | F | 1.88e+20 | 1.92229e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X132643.10+074035.4 | chandra | ccd3 | 944.539 | 544.27 | 12.3898 | 3.51997 | 0.00248669 | 0.000706474 | 4.01956 | 0.999639 | 2.80473 | 2.80473 | 0 | 8.68875 | 9.23794 | 1.81458 | -0.671645 | 0.516795 | F | F | 1.86e+20 | 3.54379e-14 | 1 | dsx |
| Report | srcpi bgdpi arf | 11 | X132601.86+073825.0 | chandra | ccd7 | 833.167 | 153.5 | 8.50649 | 4.1225 | 0.00170727 | 0.000827396 | 12.1089 | 1 | 1.60387 | 0.492 | 29.5811 | 6.23219 | 2.81818 | 5.79221 | 0.3454 | 0.511425 | A | F | 1.88e+20 | 1.4073e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X132624.73+074650.4 | chandra | ccd6 | 108.072 | 132.786 | 8.93526 | 4.1225 | 0.00179333 | 0.000827396 | 35.1162 | 1 | 0.727807 | 0.556321 | 113.523 | 4.27475 | 4 | 4.93526 | 0.10467 | 0.468371 | F | F | 1.83e+20 | 2.12268e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 8 | X132607.23+073910.2 | chandra | ccd7 | 670.833 | 245.333 | 5.70416 | 3.59808 | 0.00114484 | 0.000722143 | 10.4874 | 1 | 0.563657 | 0.492 | 63.4349 | 5.13205 | 2.92604 | 2.85208 | -0.0127998 | 0.631009 | F | F | 1.87e+20 | 9.01132e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X132650.84+074413.2 | chandra | ccd3 | 710.214 | 986.5 | 6.02512 | 3.78388 | 0.00120926 | 0.000759435 | 6.10225 | 0.999991 | 2.94286 | 1.02677 | 168.403 | 9.83825 | 2.70458 | 3.32054 | 0.102231 | 0.638723 | A | F | 1.85e+20 | 1.69607e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 7 | X132612.05+074442.3 | chandra | ccd7 | 525.3 | 920.3 | 4.91531 | 3.39792 | 0.000986514 | 0.00068197 | 16.8899 | 1 | 0.492 | 0.492 | 45 | 0.544134 | 5 | -0.0846933 | -1 | 0.975663 | F | F | 1.85e+20 | 7.42726e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X132647.83+074714.5 | chandra | ccd2 | 764.5 | 320.9 | 4.66015 | 3.39792 | 0.000935303 | 0.00068197 | 7.99383 | 0.999998 | 1.36713 | 0.783916 | 79.8384 | 9.58242 | 3.9029 | 0.757249 | -0.675011 | 0.893063 | A | F | 1.84e+20 | 1.37284e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 2 | X132642.75+074929.0 | chandra | ccd2 | 917.928 | 594.214 | 6.30241 | 3.78388 | 0.00126491 | 0.000759435 | 7.54584 | 0.999999 | 1.81156 | 1.06608 | 135.074 | 9.44207 | 4.65121 | 1.70103 | -0.46443 | 0.664517 | A | F | 1.83e+20 | 1.84369e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 3 | X132648.06+074630.9 | chandra | ccd2 | 757.375 | 232.375 | 7.01471 | 3.95804 | 0.00140787 | 0.000794388 | 7.06689 | 0.999999 | 1.95514 | 1.51671 | 144.8 | 9.4346 | 2.73726 | 4.27746 | 0.219567 | 0.583814 | F | F | 1.85e+20 | 2.04789e-14 | 1 | dx |
| Report | srcpi bgdpi arf | 5 | X132614.70+074211.7 | chandra | ccd7 | 445 | 614.25 | 3.83061 | 3.17945 | 0.000768814 | 0.000638123 | 9.30741 | 0.999999 | 0.492 | 0.492 | 142.018 | 2.20116 | 0 | 3.91531 | 1 | 1.16887 | F | F | 1.85e+20 | 5.78689e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 6 | X132618.27+074218.7 | chandra | ccd7 | 337.25 | 628.5 | 3.74592 | 3.17945 | 0.000751815 | 0.000638123 | 7.43145 | 0.999993 | 0.492 | 0.492 | 90 | 2.59489 | 2 | 0.74592 | -0.456707 | 1.20108 | F | F | 1.85e+20 | 5.6943e-15 | 1 | dx |
| Report | srcpi bgdpi arf | 1 | X132609.95+074956.5 | chandra | ccd6 | 554.5 | 511 | 3.57653 | 3.17945 | 0.000717819 | 0.000638123 | 5.49608 | 0.99992 | 0.492 | 0.492 | 26.5651 | 5.73919 | 2.66123 | 0.915307 | -0.48816 | 1.00686 | F | F | 1.83e+20 | 8.32389e-15 | 1 | dx |
counts and rate are bgd.-subtracted, based on simple spatial fitting (if done) or extracted counts from aperture otherwise (N.B., in either case aperture counts are given csv file).
cntserr, rateerr = Error on (source) counts and count rate, based on error in total counts
SNR = signal-to-noise ratio, computed using Nsrc/sqrt(Nbgd)
poisprob = Poisson probability of observing total counts given bgd. counts
sigmaj, sigmin = source extent (from detection output or spatial fitting) in units of arcsecs.
incang = position angle of source (inclination from x-axis)
cnts_soft = bgd.-subtracted counts in soft band (0.50 - 2.00 KeV, always taken directly from source aperture rather than model fitting)
cnts_hard = bgd.-subtracted counts in hard band (2.00 - 7.99 KeV, always taken directly from source aperture rather than model fitting)
hr, hr_err = hardness ratio ([cnts_hard-cnts_soft]/[cnts_hard+cnts_soft]) and error
ext = source extension flag: F = false (not extended), T = true (extended), A = asymetric (ratio of sigmaj/sigmin > 1 + x, where x = 0.5 by default)
var = variability flag: U = unknown, F = false (is not variable), T = true
N_H = Galactic column density as determined from LHEASOFT nh program
flux = flux determined from count rate using pimms (in the 0.30-8.00 keV bandpass for a power-law model with ph. index = 1.8)
vign = vignetting correction
Flags: d = detection parameters, s = simple spatial fitting parameters,
b = simple spatial fitting failed, p = poor simple spatial fit, x = extracted events parameters, t = temporal anaylsis parameters,
i = psf spatial fitting parameters, f = spectral fitting parameters,
c = source is confused, u = user-defined source, v = detected source coincident with user-defined source, r = source is in region-of-interest